Tidal Impact on Quiet-Time Polar Thermosphere Zonal Winds During Northern Winter Sudden Stratospheric Warmings

IF 2.9 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS Journal of Geophysical Research: Space Physics Pub Date : 2025-02-19 DOI:10.1029/2024JA033011
Komal Kumari, Katrina Bossert, Nicholas M. Pedatella, Denise Thorsen, Mark Conde
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Abstract

This study primarily examines the variability of zonal winds in the geomagnetic “quiet-time” (AE index < 190 nT; Kp index < 2) thermosphere over Alaska (60–75°N) during the winter months from November 2018 to February 2019, and demonstrates a correlation of the meteor radar observed zonal winds at heights 82–98 km with Scanning Doppler Imager observed zonal wind variability at heights 120 and 250 km during nighttime. Notably, over Alaska following a mid-winter sudden stratosphere warming (SSW) event, the zonal wind magnitudes on tidal timescale (difference between maximum eastward and minimum westward wind values over a 6-hr interval during nighttime) in the thermosphere experience about two-fold increase at observed thermosphere altitudes (98, 120, and 250 km). Additional validation of observational findings comes from SD-WACCM-X model simulations across solar-minimum (2017–2021) winters, including both non-SSW and SSW events (occurring in different winters). The model indicates that the SSW-induced response in zonal wind tidal magnitudes may be indistinguishable from the seasonal trend in late winter, while it is more pronounced when the seasonal variations is minimal during mid-winter months. By tidal diagnostics of zonal winds from meteor radar observations and SD-WACCM-X simulations at polar latitudes, a connection is established between the thermosphere zonal wind variations and the semidiurnal originating in the lower atmosphere following the SSW onset within the altitude range of 90–300 km (i.e., ionosphere-thermosphere region). Additionally, the study highlights the migrating solar semidiurnal tides as a major contributor in the variability in the polar thermosphere region with minor contribution from lunar semidiurnal tides.

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北方冬季平流层突然变暖期间潮汐对安静时间极地热层纬向风的影响
本研究主要考察地磁“安静时间”(AE指数<;190元;Kp指数<;2) 2018年11月至2019年2月冬季阿拉斯加(60-75°N)上空的热层,并展示了流星雷达观测到的82-98 km高度纬向风与扫描多普勒成像仪观测到的120和250 km高度夜间纬向风变化的相关性。值得注意的是,在冬季中期平流层突然变暖(SSW)事件之后的阿拉斯加上空,在观测到的热层高度(98、120和250公里),热层中潮汐时间尺度上的纬向风强度(夜间6小时间隔内最大东风值和最小西风值之差)增加了大约两倍。SD-WACCM-X模式在太阳极小期(2017-2021)冬季的模拟进一步验证了观测结果,包括非SSW和SSW事件(发生在不同的冬季)。模式表明,纬向风潮汐强度在冬末的季节变化趋势与海温的变化趋势没有明显区别,而在冬中期季节变化最小时,海温的变化趋势更为明显。通过流星雷达观测和SD-WACCM-X极纬模拟对纬向风的潮汐诊断,在90-300 km高度范围内(即电离层-热层区),建立了热层纬向风变化与起源于低层大气的半日风之间的联系。此外,该研究还强调了太阳半日潮的迁移是极地热层区变率的主要贡献者,月球半日潮的贡献较小。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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